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Table C.4

Posteriors of MCMC fittings (see text).

ab (au) Pb (yr) eb ib (deg) Ωb (deg) ωb (deg) Tpb (yr) Mb (MJup)
ac (au) Pc (yr) ec ic (deg) Ωc (deg) ωc (deg) Tpc (yr) Mc (MJup)
(M*) (d) V0 (km s−1)
NIRDIFS ≃9.0 (p) ≃20.3 (p) ≃0.01(p) 88.94 ± 0.04 − 148.31 ± 0.06 ≃47 (p) ≃8.7(p)
≃1.77(p)

NIRDIFS-GRAV 9.80 ± 0.04 22.6 ± 0.35 0.08 ± 0.01 88.99 ± 0.01 − 148.26 ± 0.02 20.4 ± 6 7.2 ± 0.4
1.835 ± 0.04

NIRDIFS-GRAV-RV 9.76 ± 0.04 22.9 ± 0.25 0.09 ± 0.01 89.01 ± 0.01 − 148.24 ± 0.02 14.3 ± 5 6.77 ± 0.3 11.1 ± 0.8
bc-corr, MG14 2.68 ± 0.02 3.0 ± 0.02 0.27 ± 0.06 89.01 ± 0.01 − 148.24 ± 0.02 − 71.9 ± 13.8 3.01 ± 0.6 7.8 ± 0.4
1.78 ± 0.03 19.4 ± 0.02 − 0.016 ± 0.004

Notes. Here, we indicate the mean ± stdev when the distribution is Gaussian, or, otherwise, the position of the peak (noted “(p)”). Tp, expressed in yr, corresponds to the time of periastron passage since JDB = 2 454 000.

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